| Start Date | Context | Status | Description |
|---|---|---|---|
| 2026-08-13 | hst_1352.pmap | latest | These WFC3 UVIS superdarks will affect all UVIS data taken from June 23, 2026 to July 13, 2026. Currently, the automated calibration pipeline and CRDS have only WFC3 UVIS drk and dkc reference files with USEAFTER dates of up to June 19, 2026. The automated pipeline should now use these reference files to perform dark subtraction on any UVIS datasets obtained between the dates above, as they represent the most accurate picture of dark current and hot pixels for this time period. These WFC3 UVIS drk and dkc files were generated using dark exposures from HST Cycle 33 CAL programs 17944 and 17947. More information regarding the method used to create the UVIS dark calibration reference files can be found in WFC3 ISR 2016-08. Additionally, the header of each reference file contains a detailed history section outlining the process, and provides a list of data used to create each file. This new bad pixel table with USEAFTER of June 23, 2026 was generated using data taken from June 23, 2026, through July 16, 2026. Currently, the Calibration Reference Data System only has WFC3 UVIS bad pixel reference tables up to a USEAFTER date of May 27, 2026. The automated pipeline should now use this reference file as the bad pixel table for any UVIS datasets obtained from June 23, 2026 to present because it represents the most accurate measure of pixel stability at the time of the science observation. These WFC3 UVIS bad pixel files were generated using 900 second dark exposures from the HST Cycle 33 daily monitoring programs 17944 and 17947. More information about the UVIS bad pixel tables is outlined in the WFC3 ISR 2018.15 and WFC3 ISR 2021.14. |
| 2026-08-12 | hst_1350.pmap | archived | The STIS TDCTAB encodes the scaling relation for STIS NUV DARKFILEs given detector temperature and date. We applied a local linear temperature fit to the last time period, and fit the residuals with a dual exponential model. This TDCTAB change quantitatively affects only data taken after 2024-06-17. |
| 2026-08-10 | hst_1349.pmap | archived | Delivery of new STIS CCD bias and dark reference files for CCD data taken between July 09 2026 through August 04 2026. The files were generated from data taken in the same time frame under STIS calibration programs 18158, and 18155. |
| 2026-08-06 | hst_1348.pmap | archived | A COS FUV LP11 DUMMY FLATFILE with the wrong optical element header keyword, OPT_ELEM, set to G130M was mistakenly delivered. This new LP11 DUMMY FLATFILE replaces the original one and has the correct optical element header keyword set to G140L. The G130M file that was delivered by mistake has also been removed from the rmap. |